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The generation of MHD waves by forced turbulence in a weakly magnetized fluidThe effect of the fluctuating buoyancy force on wave generation in a weakly magnetized plasma is considered. As expected, the efficiency of MHD wave generation is enhanced by including this force. However, it remains true that the observed variation of coronal emission at fixed spectral type cannot be accounted for by a wave generation process of the type discussed here.
Document ID
19890064537
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Rosner, R.
(Chicago, University IL, United States)
Musielak, Z. E.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 14, 2013
Publication Date
July 1, 1989
Publication Information
Publication: Astronomy and Astrophysics
Volume: 219
Issue: 1-2,
ISSN: 0004-6361
Subject Category
Solar Physics
Accession Number
89A51908
Distribution Limits
Public
Copyright
Other

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